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VIII.—Lunar Atmospheric Pressure Variations at Glasgow

Published online by Cambridge University Press:  15 September 2014

R. A. Robb  and
T. R. Tannahill
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Extract

1. In a previous communication (Robb and Tannahill, 1935) the lunar atmospheric pressure inequalities at Glasgow for days whose range of pressure was less than or equal to o·1 in. of mercury were investigated. It was found that a large first harmonic was present and that the second harmonic or semi-diurnal component had a phase angle of 285° in contradiction to the phase angle of 90° as predicted by tidal theory.

Type
Proceedings
Information
Proceedings of the Royal Society of Edinburgh , Volume 59 , 1940 , pp. 81 - 90
Copyright
Copyright © Royal Society of Edinburgh 1940

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References

References to Literature

Bartels, J., 1927. “Über die atmosphärischen Gezeiten,” Veröff. Preuss. Met. Inst., Abh. 8, Nr. 9.Google Scholar
Becker, L., 1925. “The Climatology of Glasgow,” M.O. Geophys. Mem.. no. 23.Google Scholar
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Chapman, S., and Austin, M., 1934. “The Lunar Atmospheric Tide at Buenos Ayres, 1891–1910,” Quart. Journ. Roy. Met. Soc., vol. lx, pp. 23–28.Google Scholar
Robb, R. A., and Tannahill, T. R., 1935. “The Lunar Atmospheric Pressure Inequalities at Glasgow,” Proc. Roy. Soc. Edin., vol. lv, pp. 91–96.Google Scholar